Open silcn opened 6 years ago
Do you have any estimate or even measurement data or photos from previous occasions as reference for its darkening?
I'm not an expert on this; Focas and Dollfus (http://adsabs.harvard.edu/full/1969A%26A.....2..251F) estimated in 1969 that the brightness of the backlit side of the B ring is 1/50 of the brightness of the directly illuminated side. I couldn't find any more recent data or values for the other rings in a quick search, but at least this gives a rough idea. In fact the apparent brightness of the rings varies differently from that of the planet - for instance, the rings appear much brighter very close to opposition - and this doesn't seem to be implemented either. There are presumably some good models but I'm not the person to point you in the right direction.
Thanks, that's a start. I think the ring brightness is just from ordinary Lambert reflection, there are no special effects. It might be possible to add some Oren-Nayar brightness push like for the Full Moon.
Some information that might be useful: http://bjj.mmedia.is/data/s_rings/index.html
I think the ring brightness is just from ordinary Lambert reflection, there are no special effects.
Haha, no! At the very least, there's, like for lunar regolith, an opposition surge of brightness.
This was a statement on the current state of implementation, with outlook on possible addition of an O-N effect. Feel free!
Just a feature request, sorry if someone's already suggested this. During crossings of Saturn's ring plane, there is usually a short period when Earth is on the opposite side of Saturn's rings from the Sun. When this happens, the backlit side of the rings is visible from Earth, and they appear much darker. This doesn't seem to be implemented in Stellarium yet (eg the rings should be darker in April 2025).